Babak, Stanislav and Fang, Hua and Gair, Jonathan R. and Glampedakis, Kostas and Hughes, Scott A. (2007) “Kludge” gravitational waveforms for a test-body orbiting a Kerr black hole. Physical Review D, 75 (2). Art. No. 024005. ISSN 0556-2821 http://resolver.caltech.edu/CaltechAUTHORS:BABprd07
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One of the most exciting potential sources of gravitational waves for low-frequency, space-based gravitational wave (GW) detectors such as the proposed Laser Interferometer Space Antenna (LISA) is the inspiral of compact objects into massive black holes in the centers of galaxies. The detection of waves from such “extreme mass ratio inspiral” systems (EMRIs) and extraction of information from those waves require template waveforms. The systems' extreme mass ratio means that their waveforms can be determined accurately using black hole perturbation theory. Such calculations are computationally very expensive. There is a pressing need for families of approximate waveforms that may be generated cheaply and quickly but which still capture the main features of true waveforms. In this paper, we introduce a family of such kludge waveforms and describe ways to generate them. Different kinds of kludges have already been used to scope out data analysis issues for LISA. The models we study here are based on computing a particle's inspiral trajectory in Boyer-Lindquist coordinates, and subsequent identification of these coordinates with flat-space spherical polar coordinates. A gravitational waveform may then be computed from the multipole moments of the trajectory in these coordinates, using well-known solutions of the linearised gravitational perturbation equations in flat space time. We compute waveforms using a standard slow-motion quadrupole formula, a quadrupole/octupole formula, and a fast-motion, weak-field formula originally developed by Press. We assess these approximations by comparing to accurate waveforms obtained by solving the Teukolsky equation in the adiabatic limit (neglecting GW backreaction). We find that the kludge waveforms do extremely well at approximating the true gravitational waveform, having overlaps with the Teukolsky waveforms of 95% or higher over most of the parameter space for which comparisons can currently be made. Indeed, we find these kludges to be of such high quality (despite their ease of calculation) that it is possible they may play some role in the final search of LISA data for EMRIs.
|Additional Information:||©2007 The American Physical Society (Received 4 July 2006; published 4 January 2007) We thank Kip Thorne for initially pointing us to the paper by Press, Steve Drasco for providing Teukolsky-based waveforms from generic orbits and B.S. Sathyaprakash for useful discussions. The work of J.R.G. was supported in part by NASA grants NAG5-12834 and NAG5-10707 and by St. Catharine’s College, Cambridge. K.G. acknowledges support from PPARC Grant No. PPA/G/S/2002/00038. Work of S.B. was partially supported by PPARC Grant No. PP/B500731. Work of H.F. was supported in parts by NASA grants NAG5-12834, NNG04GK98G and by NSF grants PHY-0099568 and PHY-0601459. The work of S.A.H. was supported by NASA Grants NAG5-12906 and NNG05G105G, NSF Grant No. PHY-0244424 and CAREER grant No. PHY-0449884. S.A.H. also gratefully acknowledges support from MIT’s Class of 1956 Career Development Fund.|
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|Deposited On:||05 Jan 2007|
|Last Modified:||26 Dec 2012 09:27|
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